S. J. Oliver

发表

HerMES: point source catalogues from Herschel-SPIRE observations II

Y. Roehlly, P. Norberg, L. Wang, 2013, 1312.0552.

The High Energy Universe at Sharp Focus: Chandra Science, held in conjunction with the 113th Annual Meeting of the ASP. ASP Conference Proceedings

Chris J. Willott, Richard G. McMahon, Paolo Ciliegi, 2002 .

HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4

M. Halpern, D. L. Clements, Douglas Scott, 2015, 1505.06242.

Starburst galaxies and structure in the submillimetre background towards the Hubble Deep Field

A. Efstathiou, D. H. Hughes, M. Rowan-Robinson, 1999, astro-ph/9912231.

HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations

M. Halpern, D. L. Clements, T. Babbedge, 2010, 1009.5675.

Release of the AKARI-FIS Bright Source Catalogue β-1

Takao Nakagawa, Chisato Yamauchi, Carlos Alfageme, 2009 .

Spectral energy distributions and luminosities of galaxies and AGN in the SPITZER SWIRE Legacy Survey

P. Davoodi, C. J. Lonsdale, Eduardo Gonzalez-Solares, 2004 .

A high-redshift IRAS galaxy with huge luminosityhidden quasar or protogalaxy?

M. Rowan-Robinson, C. J. Lonsdale, T. Conrow, 1991, Nature.

Herschel PEP/HerMES: the redshift evolution (0 ≤ z ≤ 4) of dust attenuation and of the total (UV+IR) star formation rate density

B. Magnelli, D. Burgarella, L. Riguccini, 2013, 1304.7000.

First results from HerMES on the evolution of the submillimetre luminosity function

D. L. Clements, T. Babbedge, M. Rowan-Robinson, 2010, 1005.2189.

HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

D. L. Clements, M. Rowan-Robinson, Douglas Scott, 2012, 1203.1925.

The topology of the IRAS Point Source Catalogue Redshift survey

M. Rowan-Robinson, Edinburgh, UK, 1998 .